Table D.1.
Strongly barred galaxies and their parameters used to study bar lanes
Galaxy | Bar | BLlength | BLshape | rmax | θbl1 | θbl2 | note |
---|---|---|---|---|---|---|---|
(B,C) | (s,l) | (c1-5) | [kpc] | [deg] | [deg] | ||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | |
NGC 1097 | C | l | 2.5 | 6.6 | 45-135 | 225-324 | |
NGC 1300 | C | l | 1.5 | 7.4 | 36-126 | 225-288 | |
NGC 1365 | C | s | 2.5 | 14.2 | 108-189 | 270-360 | |
NGC 1433 | C | s | 4.0 | 6.7 | 72-162 | 252-360 | |
NGC 1512 | C | s | 4.0 | 7.5 | 153-225 | 315-54 | |
NGC 1566 | C | s | 4.5 | 3.2 | 135-198 | 306-18 | |
NGC 1672 | C | l | 1.5 | 8.1 | 0-126 | 180-315 | |
NGC 2566 | C | N/A | 1.5 | 9.8 | 144-198 | 306-54 | |
NGC 2903 | C | l | 1.5 | 3.4 | 36-144 | 234-342 | |
NGC 3351 | C | s | 4.5 | 3.5 | 9-99 | 180-261 | b |
NGC 3507 | C | s | 1.5 | 3.1 | 90-162 | 270-342 | |
NGC 3627 | C | l | 2.0 | 3.9 | 45-126 | 234-279 | |
NGC 4303 | C | l | 3.0 | 3.1 | 63-162 | 252-342 | |
NGC 4321 | C | l | 3.5 | 4.6 | 18-126 | 198-288 | |
NGC 4535 | C | l | 2.0 | 3.5 | 126-198 | 306-36 | |
NGC 4548 | C | l | 1.0 | 5.9 | 126-216 | 333-18 | |
NGC 4579 | C | s | N/A | 4.7 | 0-108 | 198-324 | |
NGC 4941 | C | s | 4.5 | 6.8 | 72-126 | 225-360 | |
NGC 5236 | C | l | 1.5 | 2.8 | 36-126 | 198-288 | c |
NGC 5643 | C | l | 1.0 | 3.7 | 18-63 | 180-243 | |
NGC 6300 | C | l | 1.0 | 2.4 | 0-72 | 162-234 | |
NGC 7496 | C | l | 1.0 | 3.9 | 0-54 | 180-252 |
Notes. The 22 strongly barred galaxies (C) are shown with: (1) visual bar lane shape classification used for the detailed bar lane analysis presented in Section 5.4.2. We list the visual bar class (2), bar lane length class (length of the CO bar lane compared to the full bar length) BLlength (3), and bar lane shape class BLshape (4). We suggest a comparison of these data with Table 1. We list the parameters used for generating the bar lane masks: maximum radius rmax (5) which corresponds to the deprojected bar radius from Herrera-Endoqui et al. (2015) when possible, and Menendez-Delmestre et al. (2007); otherwise, we used a visual estimate based on the CO images (see text). Columns (6,7) contain the azimuthal range we use to isolate both bar lanes (θbl1, θbl2 respectively). The following symbols indicate – b: no environmental mask available and c: no literature bar lane radius available.
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